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We present measurements of the cosmic microwave background (CMB) radiationtemperature anisotropy in the multipole range 2000<ell<3000 from the QUaDtelescope's second and third observing seasons. After masking the brightestpoint sources our results are consistent with the primary LCDM expectationalone. We estimate the contribution of residual (un-masked) radio point sourcesusing a model calibrated to our own bright source observations, and a fullsimulation of the source finding and masking procedure. Including thiscontribution slightly improves the chi^2. We also fit a standard SZ template tothe bandpowers and see no strong evidence of an SZ contribution, which is asexpected for sigma_8 approx 0.8.

Small Angular Scale Measurements of the CMB Temperature Power Spectrum from QUaD